| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 75.22 | 413.53 | 49.52 | 272.55 | -17.70 | 58.19 | -33.33 | 127.42 | 0.6609 | 859.5 | 291.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 71.51 | 390.85 | 46.80 | 256.11 | -17.66 | 58.65 | -32.87 | 127.70 | 0.6559 | 1227.8 | 335.6 | |
| 0.53 | -1.00 | 0.36 | -1.00 | -18.20 | 57.13 | -34.40 | 127.15 | 0.6756 | 478.3 | 999999 | |
| 0.00 | 1.33 | 0.00 | 0.91 | -18.98 | 56.40 | -35.13 | 127.54 | 0.6885 | -503.0 | -516.2 | |
| 0.00 | 1.42 | 0.00 | 1.02 | -21.83 | 54.42 | -37.10 | 129.42 | 0.7272 | -534.0 | -543.6 | |
| 0.00 | 0.89 | 0.00 | 0.63 | -20.73 | 54.18 | -37.34 | 127.98 | 0.7221 | -419.0 | -427.0 | |
| 0.00 | 0.97 | 0.00 | 0.66 | -16.10 | 54.84 | -36.69 | 122.82 | 0.6854 | -732.0 | -594.3 | |
| 0.00 | 1.95 | 0.00 | 1.39 | -19.71 | 53.37 | -38.15 | 126.23 | 0.7232 | -730.0 | -583.8 | |
| 0.00 | 0.97 | 0.00 | 0.67 | -15.74 | 53.70 | -37.83 | 121.58 | 0.6952 | -396.0 | -356.5 | |
| 0.97 | 2.39 | 0.69 | 1.69 | -16.83 | 52.27 | -39.25 | 122.02 | 0.7166 | -852.5 | -765.2 | |
| 0.53 | 3.54 | 0.38 | 2.52 | -16.72 | 51.93 | -39.59 | 121.67 | 0.7195 | -765.2 | -517.7 | |
| 0.00 | 1.33 | 0.00 | 0.94 | -16.30 | 51.91 | -39.61 | 121.14 | 0.7173 | -894.0 | -731.9 | |
| 0.00 | 1.15 | 0.00 | 0.82 | -15.68 | 51.12 | -40.40 | 119.89 | 0.7221 | -653.0 | -557.6 | |
| 1.68 | 5.94 | 1.29 | 4.55 | -19.15 | 48.53 | -43.00 | 122.52 | 0.7663 | 714.2 | 301.3 | |
| 0.00 | 0.80 | 0.00 | 0.64 | -18.89 | 46.30 | -45.23 | 120.99 | 0.7858 | -513.0 | -430.0 | |
| Proj. U | - Projected umbra area in millionths of solar disc, negative values indicate | |
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that the umbra consists of fragmented regions which cannot be separated without losing umbral area. In this way several spots (intensity minima in the umbra) have a common umbra, e.g. -2 means that the given spot shares an umbra with spot No.2, and the common U value is indicated at spot No.2. |
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| Proj. WS | - Projected whole spot area in millionths of solar disc, negative values indicate | |
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that several umbras have a common penumbra, e.g. -7 means that the given umbra shares a penumbra with umbra No.7, and the WS value is indicated at No.7. |
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| Corr. U | - Corrected umbra area in millionths of solar hemisphere, for negative values see above | |
| Corr. WS | - Corrected whole spot area in millionths of solar hemisphere, for negative values see above | |
| B | - Heliographic latitude B; positive: North, negative: South | |
| L | - Heliographic longitude L | |
| LCM | - Longitudinal distance from the Sun's central meridian | |
| Pos. angle | - Position angle | |
| r | - Distance from the centre of Sun's disc in terms of Sun's radius | |
| MU | - Mean magnetic field within the umbra contour averaged the pixel values with sign. | |
| MP | - Mean magnetic field within the penumbra contour averaged the pixel values with sign. | |